9,298 research outputs found

    Sounds of the jungle: Re-humanizing the migrant

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    This article examines the cross-border tensions over migrant settlements dubbed ‘The Jungle’ in Calais. The Jungle, strongly associated with the unauthorized movement of migrants, became a physical entity enmeshed in discourses of illegality and violation of white suburbia. British mainstream media have either rendered the migrant voiceless or faceless, appropriating them into discourses of immigration policy and the violent transgression of borders. Through the case study, Calais Migrant Solidarity (CMS), we highlight how new media spaces can re-humanize the migrant, enabling them to tell their stories through narratives, images and vantage points not shown in the mainstream media. This reconstruction of the migrant is an important device in enabling proximity and reconstituting the migrant as real and human. This sharply contrasts with the distance framing techniques of mainstream media, which dehumanize and silence the migrant, locating the phenomenon of migration as a disruptive contaminant in civilized and ordered societies

    Flame resistant elastic elastomeric fibers

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    Development of materials to improve flame resistance of elastic elastomeric fibers is discussed. Two approaches, synthesis of polyether based urethanes and modification of synthesized urethanes with flame ratardant additives, are described. Specific applications of both techniques are presented

    Does the far-infrared/radio correlation in spiral galaxies extend to the spatial domain

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    A comparison is made between the spatial distribution of the thermal far-infrared and non-thermal radio emission of nearby spiral galaxies. This is done in an attempt to improve our understanding of the well known correlation between the integrated Infrared Astronomy Satellite (IRAS) far-infrared and radio emission of spiral galaxies, e.g., de Jong et al., 1985, Helou et al., 1986. A physical explanation for this correlation is not straight forward due to the ambiguous nature of the origin of the far-infrared and radio, and the dependence of the non-thermal radio on each galaxies' magnetic field. It is now widely believed that the infrared emission detected in the longer wavelength IRAS wavebands (less than 50 microns) arises from at least two distinct sources, e.g., Cox et al., 1986, Persson and Helou, 1987: (1) a warm (T approx. 40 K) component associated with dense dust clouds heated by embedded O and B type stars; and (2) a cooler (T approx. 20 K) component associated with diffuse dust distributed throughout the interstellar matter (ISM) heated by the interstellar radiation field. A link between the warm component and the radio via electrons originating in Type II supernovae (the ultimate fate of many of the O and B type stars responsible for the warm component) has been suggested by numerous authors. The supporting evidence is scarce and inconclusive. Researchers have attempted to provide some insight into the problem by looking at the spatial distribution of the different components in some nearby spiral galaxies, starting with the face-on spiral M51. The source of the far-infrared data is the IRAS chopped photometric channel (CPC) instrument. Warm and cold far-infrared fluxes integrated over all wavelengths and the radio intensity at two frequencies are plotted against radius. All plots are to a common resolution of 100 arcsec, the radio data originating from the Cambridge Low Frequency Synthesis Telescope (151 MHz) and the VLA (1490 MHz, from Condon, 1987). The warm and cold regions are assumed to be representedby a single galactic wide temperatures of 50 K and 20 K respectively. A dust emissivity of 1 has been assumed. The form of the plots is little effected by varying these assumptions. The radio and cold component curves appear to follow each other most closely, in contradiction to the simple OB star/type II supernovae hypothesis
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